Product Description
OWL OPTICAL WAVELENGTH LABORATORIES WT-1 WaveTester optical power meter with data storage NEW
FEATURES:
1mm photodetector with 2.5mm universal adapter (ST, SC,
and FC)
Multimode and singlemode ready
Backlit graphic LCD display with intuitive user interface
Simple 4-key operation
Power measurements shown in dBm, dB, or microwatts
Stores optical references for each wavelength to be used for
optical loss testing
Long battery life - over 250 hrs on one 9v battery
Data storage for 200 points
USB interface for continuous data logging, report printing, or
data downloading
OWL OPTICAL WAVELENGTH LABORATORIES S Reporter software for downloading data and printing
formatted fiber certification reports
Optional integrated visual fault locator (VFL)
APPLICATIONS:
The WaveTester is a high accuracy, high resolution,
microprocessor controlled, optical power meter. It has a 65dB
dynamic range, and is NIST traceable at 850, 1300, 1310,
and 1550nm, making it ideal for both singlemode and
multimode fiber testing. Additionally, it comes calibrated at
1490nm, allowing the meter to measure optical loss at the
wavelengths used in Fiber To The Home (FTTH) PON
networks.
It has an attractive handheld case with a backlit, graphic,
liquid crystal display, and 4-key keypad for easy operation. It
is offered with a 2.5mm universal fiber connector, will operate
for over 250 hours on a standard high-capacity 9v battery,
and has built-in auto shutdown.
The WaveTester will store reference values for each
wavelength to be used for optical loss measurements, and
can store up to 200 measured data points.
Stored data can be downloaded to our free OWL OPTICAL WAVELENGTH LABORATORIES S Reporter
software to produce formatted certification reports.
Optionally, the battery charging port in the WaveTester can be
replaced with a precision-coupled visual fault locator that is
optimized for fiber optics. Its high-intensity red laser allows
for fiber identification up to 1.5 kilometers away.
This optional VFL port can also be used to check for faults
within a few feet of its launch point. When the bright red light
encounters a fault, the light is deflected into the jacket,
producing a red glow at the point of the fault.